Solar proton produced neon in shergottite meteorites

Details Solar proton produced neon in shergottite meteorites Solar proton produced neon in shergottite meteorites

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994lpi....25..403g&link_type=abstract

In Lunar and Planetary Inst., The Twenty-Fifth Lunar and Planetary Science Conference. Part 1: A-G p 403-404 (SEE N94-35395 11-9

Other

Cosmochemistry, Lunar Rocks, Neon, Nuclear Interactions, Radioactive Isotopes, Shergottites, Solar Protons, Cosmology, Isotopic Labeling, Mars (Planet), Mars Surface, Meteoritic Composition

Scientific paper

Cosmogenic radionuclides produced by near-surface, nuclear interactions of energetic solar protons (approx. 10-100 MeV) were reported in several lunar rocks and a very small meteorites. We recently documented the existence and isotopic compositions of solar-produced (SCR) Ne in two lunar rocks. Here we present the first documented evidence for SCR Ne in a meteorite, ALH77005, which was reported to contain SCR radionuclides. Examination of literature data for other shergottites suggests that they may also contain a SCR Ne component. The existence of SCR Ne in shergottites may be related to a Martian origin.

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